J. Kissel

I've taken standard transfer functions of the IMs as we begin close-out of the HAM2 chamber. 
All IMs -- IM1, IM2, IM3, and IM4 -- are free of rubbing, and their dynamics look virtually identical to just-prior-to-vent measurements.
We've still got plenty of other things to do, but the IMs are ready for HAM2 door closure.

Huzzah!

Attached are the results and comparisons.

Raw data templates live in 
/ligo/svncommon/SusSVN/sus/trunk/HAUX/H1/
    IM1/SAGM1/Data/2017-12-20_2122_H1SUSIM1_M1_WhiteNoise_L_0p01to50Hz.xml
    IM1/SAGM1/Data/2017-12-20_2122_H1SUSIM1_M1_WhiteNoise_P_0p01to50Hz.xml
    IM1/SAGM1/Data/2017-12-20_2122_H1SUSIM1_M1_WhiteNoise_Y_0p01to50Hz.xml

    IM2/SAGM1/Data/2017-12-20_2124_H1SUSIM2_M1_WhiteNoise_L_0p01to50Hz.xml
    IM2/SAGM1/Data/2017-12-20_2124_H1SUSIM2_M1_WhiteNoise_P_0p01to50Hz.xml
    IM2/SAGM1/Data/2017-12-20_2124_H1SUSIM2_M1_WhiteNoise_Y_0p01to50Hz.xml

    IM3/SAGM1/Data/2017-12-20_2140_H1SUSIM3_M1_WhiteNoise_L_0p01to50Hz.xml
    IM3/SAGM1/Data/2017-12-20_2140_H1SUSIM3_M1_WhiteNoise_P_0p01to50Hz.xml
    IM3/SAGM1/Data/2017-12-20_2140_H1SUSIM3_M1_WhiteNoise_Y_0p01to50Hz.xml

    IM4/SAGM1/Data/2017-12-20_2146_H1SUSIM4_M1_WhiteNoise_L_0p01to50Hz.xml
    IM4/SAGM1/Data/2017-12-20_2146_H1SUSIM4_M1_WhiteNoise_P_0p01to50Hz.xml
    IM4/SAGM1/Data/2017-12-20_2146_H1SUSIM4_M1_WhiteNoise_Y_0p01to50Hz.xml